VLBA and EVN Imaging of GL2789

Details VLBA and EVN Imaging of GL2789 VLBA and EVN Imaging of GL2789

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..340..367v&link_type=abstract

Future Directions in High Resolution Astronomy: The 10th Anniversary of the VLBA, ASP Conference Proceedings, Vol. 340. Edited

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Radio images of maser spots in the infrared source GL2789, connected with the young stellar object V645Cyg, have been obtained as a result of the radio interferometric observations of H2O maser at 22 GHz and methanol maser at 6.7 GHz, with the VLBI arrays VLBA and EVN. It was shown that the position of the masers coincide with the optical object within 0.''2. The maser spots are located along the line North-South, and their position and radial velocity can be described by a model of the Keplerian disk.

Affiliated with

Also associated with

No associations

Rating

VLBA and EVN Imaging of GL2789 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with VLBA and EVN Imaging of GL2789, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLBA and EVN Imaging of GL2789 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1032765